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NSR database version of April 26, 2024.

Search: Author = D.Lattuada

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2023GU07      Eur.Phys.J. A 59, 65 (2023)

G.L.Guardo, T.Petruse, D.Lattuada, M.La Cognata, D.L.Balabanski, E.Aciksoz, L.Acosta, L.Capponi, D.Carbone, S.Cherubini, D.Choudhury, G.D'Agata, A.Di Pietro, P.Figuera, M.Gulino, A.I.Kilik, M.La Commara, L.Lamia, C.Matei, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, P.-A.Soderstrom, R.Sparta, A.Tumino, S.Vinals

Direct measurement of the ¹⁹F(p, α₀)¹⁶O reaction at E_cm= 0.4-0.9 using the LHASA detector array

NUCLEAR REACTIONS ¹H(¹⁹F, α), E(cm)=0.4-0.9 MeV; measured reaction products, Eα, Iα; deduced σ(θ), S-factor. Comparison with NACRE compilation, available data. INFN-Laboratori Nazionali del Sud, Catania (Italy).

doi: 10.1140/epja/s10050-023-00957-1
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Data from this article have been entered in the XUNDL database. For more information, click here.

2023TU05      Commun. Phys. 6, 106 (2023)

A.Tumino, G.G.Rapisarda, M.La Cognata, A.Oliva, A.Kievsky, C.A.Bertulani, G.D'Agata, M.Gattobigio, G.L.Guardo, L.Lamia, D.Lattuada, R.G.Pizzone, S.Romano, M.L.Sergi, R.Sparta, M.Viviani

Coulomb-free ¹S_o p - p scattering length from the quasi-freep p + d → p + p + n reaction and its relation to universality

NUCLEAR REACTIONS ²H(p, 2p), E(cm)<1 MeV; analyzed available data; deduced p-p scattering σ, σ(θ), scattering length and effective range from a Bayesian approach analysis.

doi: 10.1038/s42005-023-01221-0
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2022LA01      Phys.Lett. B 826, 136917 (2022)

M.La Cognata, S.Palmerini, P.Adsley, F.Hammache, A.Di Pietro, P.Figuera, R.Alba, S.Cherubini, F.Dell'Agli, G.L.Guardo, M.Gulino, L.Lamia, D.Lattuada, C.Maiolino, A.Oliva, R.G.Pizzone, P.M.Prajapati, S.Ramano, D.Santonocito, R.Sparta, M.L.Sergi, A.Tumino

Exploring the astrophysical energy range of the ²⁷Al(p, α)²⁴Mg reaction: A new recommended reaction rate

NUCLEAR REACTIONS ²H(²⁷Al, α²⁴Mg)¹NN, E<1.5 MeV; measured reaction products. ²⁸Si, ²⁴Mg; deduced σ(θ, E), strengths of the levels, astrophysical reaction rates. The indirect Trojan Horse method (THM), INFN-LNS Tandem accelerator (Catania, Italy).

doi: 10.1016/j.physletb.2022.136917
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Data from this article have been entered in the XUNDL database. For more information, click here.

2022LA06      Phys.Rev. C 105, 044618 (2022)

H.Y.Lan, W.Luo, Y.Xu, D.L.Balabanski, G.L.Guardo, M.La Cognata, D.Lattuada, C.Matei, R.G.Pizzone, T.Rauscher, J.L.Zhou

Feasibility of studying astrophysically important charged-particle emission with the variable energy γ-ray system at the Extreme Light Infrastructure--Nuclear Physics facility

NUCLEAR REACTIONS ²⁹Si, ⁴⁷Ti, ⁵⁶Fe, ⁷³Ge, ⁷⁴Se, ⁸⁴Sr, ⁹¹Zr, ⁹⁵Mo, ^96,98Ru, ¹⁰²Pd, ¹⁰⁶Cd, ^115,117,119Sn, ¹³²Ba, ¹⁴³Nd(γ, p), (γ, np), E<30 MeV; ⁵⁰V, ⁶⁷Zn, ⁸⁷Sr, ¹⁰⁷Ag, ^113,115In, ¹¹⁹Sn, ^123,125Te, ^149,154Sm, ^{155,156,157,158,160}Gd, ²⁰⁸Pb(γ, α), (γ, nα), E<30 MeV; calculated inclusive and exclusive σ(E), population of the particular excited states, energy spectra of ejectiles. TALYS-1.9 calculations with various combinations of level densities, strength functions and optical potentials available in the code.Investigated the feasibility of studying the reactions of astrophysical interest with ELI-NP facility infrastructure. Simulated achievable yields.

doi: 10.1103/PhysRevC.105.044618
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2022LA14      Astrophys.J. 941, 96 (2022)

M.La Cognata, S.Palmerini, P.Adsley, F.Hammache, A.Di Pietro, P.Figuera, F.Dell'Agli, R.Alba, S.Cherubini, G.L.Guardo, M.Gulino, L.Lamia, D.Lattuada, C.Maiolino, A.Oliva, R.G.Pizzone, P.M.Prajapati, G.G.Rapisarda, S.Romano, D.Santonocito, R.Sparta, M.L.Sergi, A.Tumino, P.Ventura

A New Reaction Rate of the ²⁷Al(p/α)²⁴Mg Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for ²⁷Al Yields of Intermediate-mass Stars

NUCLEAR REACTIONS ²H(²⁷Al, α²⁴Mg), E=80 MeV; measured reaction products. ²⁸Si, ²⁴Mg; deduced σ(θ), σ(θ, E), resonance strengths. Comparison with Monte Carlo code RatesMC. Indirect Trojan Horse Method (THM), the INFN-LNS Tandem (Catania, Italy).

doi: 10.3847/1538-4357/ac9c5e
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Data from this article have been entered in the XUNDL database. For more information, click here.

2021SP02      Eur.Phys.J. A 57, 20 (2021)

C.Spitaleri, S.Typel, C.A.Bertulani, A.M.Mukhamedzhanov, T.Kajino, M.Lattuada, A.Cvetinovic, S.Messina, G.L.Guardo, N.Soic, M.Milin, S.S.Perrotta, C.Li, P.Colovic, G.D'Agata, D.Dell'Aquila, C.G.Fatuzzo, M.Gulino, S.Q.Hou, M.La Cognata, D.Lattuada, D.Nurkic, R.Popocovski, N.Skukan, S.Szilner, O.Trippella, M.Uroic, N.Vukman

The ³He + ⁵He → α+α reaction below the Coulomb barrier via the Trojan Horse Method

NUCLEAR REACTIONS ⁹Be(³He, 2α), E=4 MeV; ³He(⁵He, α), E(cm)<1 Mev; measured reaction products, Eα, Iα; deduced two α-particles σ(θ, E), σ(θ). Comparison with theoretical calculations, Trojan Horse Method (THM).

doi: 10.1140/epja/s10050-020-00324-4
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD1037.

2021SP03      Eur.Phys.J. A 57, 170 (2021)

R.Sparta, L.Lamia, M.La Cognata, C.Spitaleri, G.G.Rapisarda, G.L.Guardo, S.Cherubini, G.D'Agata, A.Di Pietro, P.Figuera, M.Gulino, D.Lattuada, M.Lattuada, S.Palmerini, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino, S.Typel

¹⁰B(n, α₀)⁷Li and ¹⁰B(n, α₁)⁷Li reactions measured via Trojan Horse Method

NUCLEAR REACTIONS ²H(¹⁰B, α⁷Be), E=28 MeV; measured reaction products, Eα, Iα; deduced momentum distribution for the spectator particle, σ(θ), σ(E), ¹⁰B(n, α) σ using the Trojan Horse Method.

doi: 10.1140/epja/s10050-021-00481-0
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2020MU07      Phys.Rev. C 101, 055801 (2020)

M.Munch, C.Matei, S.D.Pain, M.T.Febbraro, K.A.Chipps, H.J.Karwowski, C.Aa.Diget, A.Pappalardo, S.Chesnevskaya, G.L.Guardo, D.Walter, D.L.Balabanski, F.D.Becchetti, C.R.Brune, K.Y.Chae, J.Frost-Schenk, M.J.Kim, M.S.Kwag, M.La Cognata, D.Lattuada, R.G.Pizzone, G.G.Rapisarda, G.V.Turturica, C.A.Ur, Y.Xu

Measurement of the ⁷Li(γ, t)⁴He ground-state cross section between E_γ = 4.4. and 10 MeV

NUCLEAR REACTIONS ⁷Li(γ, t), E=4.4-10 MeV from High Intensity Gamma-ray Source (HIγS) at TUNL; measured E(t), I(t), Eα, Iα, Eγ and Iγ, αt-coin, ground state σ(E) using the SIDAR silicon detector array. ³H(α, γ), E(cm)=0-7 MeV; deduced astrophysical S-factor from R-matrix analysis. Comparison with model predictions, and with previous experimental results. Relevance to primordial Li problem and the mirror α-capture reactions.

doi: 10.1103/PhysRevC.101.055801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetL0260. Data from this article have been entered in the XUNDL database. For more information, click here.

2020PI11      Eur.Phys.J. A 56, 199 (2020)

R.G.Pizzone, C.Spampinato, R.Sparta, M.Couder, W.Tan, V.Burjan, G.D'Agata, G.L.Guardo, M.La Cognata, L.Lamia, J.Mrazek, S.Palmerini, S.Typel, A.Tumino, M.Wiescher, S.Anguilar, D.Bardayan, D.Blankstein, L.Boccioli, L.Callahan, S.M.Cha, K.Y.Chae, A.M.Clark, B.Frentz, M.R.Hall, A.Gula, S.Henderson, R.Kelmar, M.S.Kwag, I.Indelicato, M.La Commara, D.Lattuada, Q.Liu, J.Long, M.Mazzocco, A.Majumdar, S.McGuinness, A.Nelson, A.A.Oliva, P.O'Malley, P.M.Prajapati, G.G.Rapisarda, S.Romano, M.L.Sergi, C.Seymour, M.Skulski, C.Spitaleri, J.Wilkinson

Indirect measurement of the ³He(n, p)³H reaction cross section at Big Bang energies

NUCLEAR REACTIONS ²H(³He, pt), E=9 MeV; measured reaction products, Ep, Ip; deduced σ for ³He(n, p) reaction using the Trojan Horse Method (THM).

doi: 10.1140/epja/s10050-020-00212-x
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset14716.

2020SO26      Commun. Phys. 11, 3242 (2020)

P.-A.Soderstrom, L.Capponi, E.Aciksoz, T.Otsuka, N.Tsoneva, Y.Tsunoda, D.L.Balabanski, N.Pietralla, G.L.Guardo, D.Lattuada, H.Lenske, C.Matei, D.Nichita, A.Pappalardo, T.Petruse

Electromagnetic character of the competitive γγ/γ-decay from ^137mBa

RADIOACTIVITY ¹³⁷Cs(β^-), ¹³⁷Ba(IT); measured decay products, Eγ, Iγ, γ-γ-coin.; deduced γ-ray energies, widths and nuclear static dipole polarisabilities, angular correlation of the two photons emitted in the double-γ decay, Energy-sharing distribution for the two photons in the double-γ decay, an improved value on the double-photon versus single-photon branching ratio. Comparison with calculations. CeBr₃ detectors from ELIGANT, the ELI Gamma Above Neutron Threshold (ELIGANT) detector system.

doi: 10.1038/s41467-020-16787-4
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Data from this article have been entered in the XUNDL database. For more information, click here.

2020SP02      Eur.Phys.J. A 56, 18 (2020)

C.Spitaleri, M.Lattuada, A.Cvetinovic, N.Soic, M.Milin, P.Colovic, G.D'Agata, D.Dell'Aquila, G.L.Guardo, M.Gulino, O.Trippella, M.La Cognata, L.Lamia, D.Lattuada, C.Li, S.Messina, D.Nurkic, S.S.Perrotta, R.G.Pizzone, R.Popoconski, S.Romano, N.Skukan, R.Sparta, S.Szilner, M.Uroic, N.Vukman

Study of the quasi-free ³He + ⁹Be → 3α reaction for the Trojan Horse Method

doi: 10.1140/epja/s10050-020-00026-x
Citations: PlumX Metrics

2019GU32      Eur.Phys.J. A 55, 211 (2019)

G.L.Guardo, C.Spitaleri, L.Lamia, R.Spartá, N.Carlin, S.Cherubini, G.Gimenez Del Santo, I.Indelicato, M.La Cognata, D.Lattuada, S.Messina, M.Munhoz, S.S.Perrotta, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, F.A.Souza, A.Szanto de Toledo, S.Tudisco, A.Tumino

The ¹⁰B(n, α)⁷Li cross sections at ultra-low energy through the Trojan Horse Method applied to the ²H(¹⁰B, α⁷Li)¹H

doi: 10.1140/epja/i2019-12914-0
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset31824. Data from this article have been entered in the XUNDL database. For more information, click here.

2019LA08      Phys.Rev. C 99, 034301 (2019)

M.La Cognata, M.Fisichella, A.Di Pietro, P.Figuera, V.Z.Goldberg, S.Cherubini, J.P.Fernandez-Garcia, M.Gulino, L.Lamia, D.Lattuada, M.Lattuada, R.G.Pizzone, G.G.Rapisarda, S.Romano, R.Sparta, C.Spitaleri, D.Torresi, A.Tumino, M.Zadro

Observation of ¹⁵N α resonant structures in ¹⁹F using the thick target in inverse kinematics scattering method

NUCLEAR REACTIONS ⁴He(¹⁵N, α), E=40.23 MeV; measured Eα, Iα, differential σ(θ) using ΔE-E silicon telescopes for α detection and surface barrier detectors for ¹⁵N-like recoils at the LNL-Catania Tandem accelerator facility. ¹⁹F; deduced levels, resonances, J, π, α-widths, proton widths and potential α-cluster states using R-matrix analysis using AZURE2 code. Comparison with previous experimental data, and with literature data for mirror nucleus ¹⁹Ne. Relevance to models of stars in different evolutionary stages, such as the asymptotic giant branch (AGB) stars asymptotic giant branch (AGB).

doi: 10.1103/PhysRevC.99.034301
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2432. Data from this article have been entered in the XUNDL database. For more information, click here.

2018LA14      Phys.Rev. C 98, 054601 (2018)

H.Y.Lan, Y.Xu, W.Luo, D.L.Balabanski, S.Goriely, M.La Cognata, C.Matei, A.Anzalone, S.Chesnevskaya, G.L.Guardo, D.Lattuada, R.G.Pizzone, S.Romano, C.Spitaleri, A.Taffara, A.Tumino, Z.C.Zhu

Determination of the photodisintegration reaction rates involving charged particles: Systematic calculations and proposed measurements based on the facility for Extreme Light Infrastructure--Nuclear Physics

NUCLEAR REACTIONS ⁷⁴Se, ⁸⁴Sr, ⁹²Mo, ⁹⁶Ru, ¹⁰²Pd, ¹⁰⁶Cd, ¹¹²Sn, ¹²⁰Te(γ, p), E(cm)=8-20 MeV; ⁷⁴Se, ⁸⁴Sr, ⁹²Mo, ⁹⁶Ru, ¹⁰²Pd, ¹⁰⁶Cd, ¹¹²Sn, ¹²⁰Te, ¹³²Ba, ¹⁴⁴Sm, ¹⁴⁸Gd, ¹⁸⁴Os(γ, α), E(cm)=6-20 MeV; calculated σ(E), proton and α-particle spectra and yields, Gamow windows at T₉=2.5 and minimum required energies of the incident γ beam satisfying the measurable criteria of the minimum detectable limit and the particle identification. Z=10-100, N=10-160; calculated ratios of the (γ, p) and (γ, α) astrophysical reaction rates at T₉=2.5 for 3000 targets of stable and proton-rich nuclei. Optical potential model calculations using Woods-Saxon and microscopic folding JLMB optical model potentials. Relevance to p-process nucleosynthesis, and the measurements of six (γ, p) and eight (γ, α) reactions based on the γ-beam facility and the Extreme Light Infrastructure Silicon Strip Array (ELISSA) for the detection of charged particles at ELI-NP, Bucharest facility.

doi: 10.1103/PhysRevC.98.054601
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2016LA10      Phys.Rev. C 93, 045808 (2016)

D.Lattuada, M.Barbarino, A.Bonasera, W.Bang, H.J.Quevedo, M.Warren, F.Consoli, R.De Angelis, P.Andreoli, S.Kimura, G.Dyer, A.C.Bernstein, K.Hagel, M.Barbui, K.Schmidt, E.Gaul, M.E.Donovan, J.B.Natowitz, T.Ditmire

Model-independent determination of the astrophysical S factor in laser-induced fusion plasmas

NUCLEAR REACTIONS ²H(d, n)³He, ³He(d, p)⁴He, E(cm)=5-500 keV; measured deuterium ion energy density distribution from time-of-flight, neutron yields from d+d fusion, angular distribution of neutrons, yield of 14.7-MeV protons using various scintillation detectors; deduced model-independent astrophysical factor S(E). Laser-induced fusion plasmas using Texas Petawatt Laser (TPW). Comparison with previous experimental data. Relevance to primordial abundances in Big Bang nucleosynthesis (BBN) models, and plasma physics.

doi: 10.1103/PhysRevC.93.045808
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2236.